Nucleosynthesis in Core-Collapse Supernovae

Fröhlich, Carla and Curtis, Sanjana and Ebinger, Kevin and Liebendörfer, Matthias and Perego, Albino and Thielemann, Friedrich-Karl. (2019) Nucleosynthesis in Core-Collapse Supernovae. In: Nuclei in the Cosmos XV, 219. Cham, pp. 99-103.

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Official URL: https://edoc.unibas.ch/75114/

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Core-collapse supernovae (CCSNe) are one of the most important nucleosynthesis sites and they hold a key role in the evolution of galaxies. In the explosion, CCSNe eject freshly synthesized iron-group nuclei from explosive burning alongside of intermediate mass elements (from hydrostatic and explosive burning), and carbon and oxygen from the pre-explosion evolution. In the neutrino-driven wind, nuclei beyond the iron group can be synthesized under neutron-rich conditions (weak r-process) and proton-rich conditions (νp-process). The signature of CCSN nucleosynthesis can be observed in the atmospheres of the oldest stars. Here, we will compare the nucleosynthesis from different progenitor models exploded with the PUSH method in spherical symmetry.
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Thielemann, Friedrich-Karl and Liebendörfer, Matthias
Item Type:Conference or Workshop Item, refereed
Conference or workshop item Subtype:Conference Paper
Series Name:Springer Proceedings in Physics
Note:Publication type according to Uni Basel Research Database: Conference paper
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Last Modified:23 Sep 2020 15:15
Deposited On:10 Mar 2020 10:46

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